PIRSA:21110000

Video URL

https://pirsa.org/21110000

Weak lensing: globally optimal estimator and a new probe of the high-redshift Universe

Maniyar, A. (2021). Weak lensing: globally optimal estimator and a new probe of the high-redshift Universe . Perimeter Institute for Theoretical Physics. https://pirsa.org/21110000

Maniyar, Abhishek. Weak lensing: globally optimal estimator and a new probe of the high-redshift Universe . Perimeter Institute for Theoretical Physics, Nov. 02, 2021, https://pirsa.org/21110000 

          @misc{ scivideos_PIRSA:21110000,
            doi = {10.48660/21110000},
            url = {https://pirsa.org/21110000},
            author = {Maniyar, Abhishek},
            keywords = {Cosmology},
            language = {en},
            title = {Weak lensing: globally optimal estimator and a new probe of the high-redshift Universe },
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2021},
            month = {nov},
            note = {PIRSA:21110000 see, \url{https://scivideos.org/pirsa/21110000}}
          }

Abhishek Maniyar New York University (NYU)

Talk numberPIRSA:21110000
DOI10.48660/21110000
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

In recent years, weak lensing of the cosmic microwave background (CMB) has emerged as a powerful tool to probe fundamental physics. The prime target of CMB lensing surveys is the lensing potential, which is reconstructed from observed CMB temperature T and polarization E and B fields. In this talk, I will show that the classic Hu-Okamoto (HO02) estimator used for the lensing potential reconstruction is not the absolute optimal lensing estimator that can be constructed out of quadratic combinations of T, E and B fields. Instead, I will derive the global-minimum-variance (GMV) lensing quadratic estimator and show explicitly that the HO02 estimator is suboptimal to the GMV estimator.

Rapidly expanding field of the line intensity mapping (LIM) promises to revolutionise our understanding of the galaxy formation and evolution. Although primarily a tool for galaxy astrophysics, LIM technique can be used as a cosmological probe and I will point out one such application in rest of the talk. I will show that a linear combination of lensing maps from the cosmic microwave background (CMB) and from line intensity maps (LIMs) allows to exactly null the low-redshift contribution to CMB lensing, and extract only the contribution from the Universe from/beyond reionization. This would provide a unique probe of the Dark Ages, complementary with 21 cm. I will quantify the interloper bias (which is a key hurdle to LIM techniques) to LIM lensing for the first time, and derive a "LIM-pair" estimator which nulls it exactly.

In the end, I will show some results for prospects of observing the Doppler boosted CIB emission and its applications.